Results 91 to 100 of about 12,099 (232)
Measurements of Stellar Properties through Asteroseismology: A Tool for Planet Transit Studies
Oscillations occur in stars of most masses and essentially all stages of evolution. Asteroseismology is the study of the frequencies and other properties of stellar oscillations, from which we can extract fundamental parameters such as density, mass ...
Bedding +7 more
core +1 more source
Asteroseismology of 16000 Kepler Red Giants: Global Oscillation Parameters, Masses, and Radii
The Kepler mission has provided exquisite data to perform an ensemble asteroseismic analysis on evolved stars. In this work we systematically characterize solar-like oscillations and granulation for 16,094 oscillating red giants, using end-of-mission ...
Bedding, Timothy R. +6 more
core +1 more source
Listening to the heartbeat: Tidal Asteroseismology in action [PDF]
Zhao Guo
openalex +1 more source
Context. The synergy between close binary stars and asteroseismology enables constraints on mass-transfer episodes and their consequences for internal structure, rotation profiles, and oscillation modes. Aims.
Wu Tao, Guo Zhao, Li Yan
doaj +1 more source
A 20-Second Cadence View of Solar-Type Stars and Their Planets with TESS: Asteroseismology of Solar Analogs and a Re-characterization of pi Men c [PDF]
Daniel Huber +52 more
openalex +1 more source
An asteroseismology explorer [PDF]
In response to a NASA opportunity, a proposal has been made to study the concept of an Asteroseismology Explorer (ASE). The goal of the ASE would be to measure solar-like oscillations on many (perhaps hundreds) of stars during a 1-year mission, including many members of open clusters.
Brown, T. M., Cox, A. N.
openaire +1 more source
Editorial: White Dwarfs in the Age of the Great Collaborations
Alejandro Hugo Córsico +6 more
doaj +1 more source
Over 2,000 stars were observed for 1 month with a high enough cadence in order to look for acoustic modes during the survey phase of the Kepler mission. Solar-like oscillations have been detected in about 540 stars.
Savita Mathur +10 more
doaj +1 more source
21 pages; This is a pre-print of an invited chapter for the Encyclopedia of Astrophysics (edited by I. Mandel, section editor F.R.N.
Bowman, Dominic M., Bugnet, Lisa
openaire +2 more sources
Editorial: Challenges of asteroseismology in the era of space missions
Javier Pascual-Granado +3 more
doaj +1 more source

